The escape velocity from the surface of a planet of mass M and radius R is given by
Ve=√2GMR
⇒Ve=√2√GMR2×R
putting the value, g=GMR2
∴Ve=√2√gR
So, Ve∝√gR
⇒Ve1Ve2=√g1√g2×√R1√R2
⇒Ve1Ve2=√(9.63.2)×√(72002400)=√3×√3
⇒Ve1:Ve2=3:1
Accepted answers : 3 , 3.0 , 3.00
Why this question: To make students to understand the dependence of escape velocity on acceleration due to gravity and radius of a planet.